A photometric study of contact binary XY Boo

Details A photometric study of contact binary XY Boo A photometric study of contact binary XY Boo

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.107..347a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 107, no. 2, Dec. 1984, p. 347-356. Research supported by the Japan Interna

Astronomy and Astrophysics

Astrophysics

5

Astronomical Photometry, Binary Stars, Variable Stars, Light Curve, Radii, Stellar Mass, Stellar Motions

Scientific paper

The contact binary XY Boo is observed photoelectrically, and variations of the orbital period and the light curves are indicated. New BV light curves and those of Binnendijk (1971) and Winkler (1977) are analysed by use of the light curve synthesis method. Combining the derived photometric elements with the spectroscopic elements of McLean and Hilditch (1983), the authors obtain values of the masses and the radii of the components of the system.

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